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Game_Minds t1_j0gtonc wrote

Well no. If we had no other ways of determining the mass of the sun, then maybe. But we can do gravitational lensing measurements and things, and the whole eclipse thing, and fusion doesn't happen at earth sized masses, etc etc etc. There are many ways to determine that the sun is millions of times the size of earth, and that the system is spinning, and put both together and we are orbiting the sun

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aaeme t1_j0h75op wrote

The hypothetical scenario is something like if we always lived in caverns miles beneath the surface so didn't even know the sun existed. Could we tell by local experiments that the earth was in motion and in orbit and the metrics of that orbit?

I think in theory we could from tidal forces and we'd notice a periodicity of a year for those and could in theory work the rest out.

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pelican_chorus t1_j0ha7gb wrote

But isn't an orbiting body in free-fall? And a body in free-fall can't feel the force of the body it's falling towards, right? That was my point. Isn't it an inertial frame?

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aaeme t1_j0hb31e wrote

At an infinitesimal point yes but across a volume tidal forces exist. There would be a slight stretching in the direction of the Sun and squeezing tangential to the Sun.

Across a year those forces would rotate 360° and not uniformly (we could calculate the eccentricity of the elliptical orbit from that).

Edit: measuring all that would be a lot more difficult because the earth is spinning so would have to figure that out so we can subtract the effects of that on our measurements.

It's hard to imagine how any species could properly understand physics well enough to do this without seeing the night sky so perhaps a better mind experiment is if a scientist got teleported to a sealed windowless box on a random planet somewhere in the universe could they tell by measurement whether the planet was in orbit around a star or not and the details of that orbit. I'm 99% sure they could from tidal forces and possibly by other means too.

Edit 2: another way to tell would be from the time-dilation differential from one side of the room to the other. A clock slightly deeper in the star's gravity well would run slightly slower.

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